Robots Refurbish Space Shuttle Hardware USBI

USBI, a division of United Technologies Corporation (UTC ), was awarded a contract by the National Aeronautics and Space Administration (NASA) to refurbish the non-motor sections (nosecap, frustum, forward skirt, and aft skirt) of the Solid Rocket Boosters (SRB) used in the space shuttle program. As NASA\u27s major contractor for processing and refurbishment of the SRB\u27s, our company has successfully refurbished all the SRB\u27s flight hardware to date. The planned insulation refurbishment process of the SRB\u27s consists of thermal protection system (TPS) removal; surface preparation; reapplication of Marshall Sprayable Ablative (MSA-2), a thermal ablative material developed at Marshall Space Flight Center; and topcoat spraying of Hypalon paint to seal the ablative material. In the past, refurbishment of the SRB\u27s was done by hand at the Vehicle Assembly Building (VAB). This process was slow and tedious, and introduced personnel to potentially hazardous working environments. A means of reducing costs and providing enhanced quality assurance was desired. Therefore, the need arose to implement a degree of automation to the refurbishment process. The introduction of a new automated process system would reduce the manual labor element, limiting the need for personnel to come in direct contact with hazardous materials. And because of the reliability and accuracy of robotics, NASA would be assured of receiving the highest possible quality product , at the lowest cost

Predicting Dust Distribution in Protoplanetary Discs

We present the results of three-dimensional numerical simulations that include the effects of hydrodynamical forces and gas drag upon an evolving dusty gas disk. We briefly describe a new parallel, two phase numerical code based upon the smoothed particle hydrodynamics (SPH) technique in which the gas and dust phases are represented by two distinct types of particles. We use the code to follow the dynamical evolution of a population of grains in a gaseous protoplanetary disk in order to understand the distribution of grains of different sizes within the disk. Our ``grains'' range from metre to submillimetre in size.Comment: 2 pages, LaTeX with 1 ps figure embedded, using newpasp.sty (supplied). To appear in the proceedings of the XIXth IAP colloquium "Extrasolar Planets: Today and Tomorrow" held in Paris, France, 2003, June 30 -- July 4, ASP Conf. Se

The Design and Development of Enhanced Thermal Desorption Products

This research study is based on a knowledge-transfer collaboration between The National Centre for Product Design and Development Research (PDR) and Markes International Ltd. The aim of the two-year collaboration has been to implement design tools and techniques for the development of enhanced thermal desorption products. Thermal desorption is a highly-specialised technique for the analysis of trace-level volatile organic compounds. This technique allows minute quantities of these compounds to be measured; however, there is an increasing demand from customers for greater sensitivity over a wider range of applications, which means new design methodologies need to be evaluated. The thermal desorption process combines a number of disparate chemical, thermal and mechanical disciplines, and the major design constraints arise from the need to cycle the sample through extremes in temperature. Following the implementation of a comprehensive product design specification, detailed design solutions have been developed using the latest 3D CAD techniques. The impact of the advanced design techniques is assessed in terms of improved product performance and reduced development times, and the wider implications of new product development within small companies are highlighted. 

Assigning Collaborative Learning Pairs Based on Personality Testing

This study, conducted at Buford Middle School, examined the effects of using personality tests to create student learning pairs. Four seventh grade classes were examined. The content, instruction, and instructor were the same for all classes. Three of four classes had students grouped in learning pairs based on the results of personality tests. The control group consisted of students grouped randomly into learning pairs. A teacher developed exam similar to the Georgia Criterion Referenced Competency Test (CRCT) for Life Science was used as the pretest and the CRCT was used as the posttest. No significant differences were found; however, specific student populations did exhibit gains in their posttest scores

Bright source of spectrally uncorrelated polarization-entangled photons with nearly single-mode emission

We present results of a bright polarization-entangled photon source operating at 1552 nm via type-II collinear degenerate spontaneous parametric down-conversion in a periodically poled potassium titanyl phosphate crystal. We report a conservative inferred pair generation rate of 123,000 pairs/s/mW into collection modes. Minimization of spectral and spatial entanglement was achieved by group velocity matching the pump, signal and idler modes and through properly focusing the pump beam. By utilizing a pair of calcite beam displacers, we are able to overlap photons from adjacent down-conversion processes to obtain polarization-entanglement visibility of 94.7 +/- 1.1% with accidentals subtracted.Comment: 4 pages, 7 color figures. Revised manuscript includes the following changes: corrected pair generation rate from 44,000/s/mW pump to 123,000/s/mW pump; replaced Fig. 1b to enhance clarity; minor alterations to the title, abstract and introduction; grammatical correction

Relativistic Proton Production During the 14 July 2000 Solar Event: The Case for Multiple Source Mechanisms

Protons accelerated to relativistic energies by transient solar and interplanetary phenomena caused a ground-level cosmic ray enhancement on 14 July 2000, Bastille Day. Near-Earth spacecraft measured the proton flux directly and ground-based observatories measured the secondary responses to higher energy protons. We have modelled the arrival of these relativistic protons at Earth using a technique which deduces the spectrum, arrival direction and anisotropy of the high-energy protons that produce increased responses in neutron monitors. To investigate the acceleration processes involved we have employed theoretical shock and stochastic acceleration spectral forms in our fits to spacecraft and neutron monitor data. During the rising phase of the event (10:45 UT and 10:50 UT) we find that the spectrum between 140 MeV and 4 GeV is best fitted by a shock acceleration spectrum. In contrast, the spectrum at the peak (10:55 UT and 11:00 UT) and in the declining phase (11:40 UT) is best fitted with a stochastic acceleration spectrum. We propose that at least two acceleration processes were responsible for the production of relativistic protons during the Bastille Day solar event: (1) protons were accelerated to relativistic energies by a shock, presumably a coronal mass ejection (CME). (2) protons were also accelerated to relativistic energies by stochastic processes initiated by magnetohydrodynamic (MHD) turbulence.Comment: 38 pages, 9 figures, accepted for publication in the Astrophysical Journal, January, 200